Individual power density spectra of Swift gamma-ray bursts

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Volume 589 (May 2016)

A&A, 589 (2016) A98

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Table 4

Best–fitting model along with means and standard deviations of the parameters’ posterior distributions for each GRB of the sample of 215 events in the 50−150 keV energy band.

GRB	Model	log N	log f_b	α	B	p(T_R) ^a	p _AD ^b	p _KS ^c
			(Hz)

050117	PL	−0.165 ± 0.051	NA	1.247 ± 0.059	1.944 ± 0.029	0.424	0.594	0.857
050124	PL	0.861 ± 0.116	NA	2.245 ± 0.333	1.811 ± 0.140	0.643	0.520	0.460
050128	PL	0.529 ± 0.046	NA	1.426 ± 0.098	1.785 ± 0.071	0.054	0.455	0.510
050219A	PL	−1.533 ± 0.375	NA	2.684 ± 0.354	1.986 ± 0.055	0.466	0.993	0.987
050219B	PL	0.112 ± 0.054	NA	1.637 ± 0.072	1.897 ± 0.039	0.089	0.972	0.963
050306	PL	−1.229 ± 0.203	NA	1.505 ± 0.145	2.010 ± 0.024	0.237	0.642	0.863
050315	PL	−1.769 ± 0.332	NA	1.849 ± 0.225	1.986 ± 0.026	0.559	0.874	0.679
050326	BPL	3.226 ± 0.176	−0.979 ± 0.110	2.437 ± 0.138	1.884 ± 0.053	0.570	0.833	0.975
050401	PL	0.236 ± 0.068	NA	1.561 ± 0.106	1.986 ± 0.061	0.378	0.971	0.820

Notes.

^(a)

p(T_R) is the significance associated with statistic T_R.

^(b)

p_AD is the significance of the Anderson-Darling test.

^(c)

p_KS is the significance of the Kolmogorov-Smirnov test.

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